Solar Photosphere: Intranetwork and Turbulent Magnetic Fields

Details Solar Photosphere: Intranetwork and Turbulent Magnetic Fields Solar Photosphere: Intranetwork and Turbulent Magnetic Fields

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke2009s&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 2009. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Sun, Solar Atmosphere

Scientific paper

The names `intranetwork' and `turbulent magnetic fields' are used to represent the solar magnetic fields of mixed polarities at the smallest scales of the spatial spectrum. Since the spatial separation of the opposite polarities is small, and since the magnetic flux of each small-scale magnetic element is tiny, they can only be made partly visible in `deep' magnetograms obtained with both high sp...

Affiliated with

Also associated with

No associations

Rating

Solar Photosphere: Intranetwork and Turbulent Magnetic Fields does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Solar Photosphere: Intranetwork and Turbulent Magnetic Fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar Photosphere: Intranetwork and Turbulent Magnetic Fields will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1151551